4.3 Article

The evolution of black hole states

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ASTROPHYSICS AND SPACE SCIENCE
卷 300, 期 1-3, 页码 107-117

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SPRINGER
DOI: 10.1007/s10509-005-1197-4

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accretion; accretion disks; black hole physics; X-rays; stars; X-rays; binaries

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We discuss the evolution of black hole transients on the basis of a few systems that were intensively observed with the Rossi X-ray Timing Explorer (rxte). We focus on the global evolution and the observed state transitions. Rather than giving a numerical recipe for classifying observations, we try to identify times during outbursts at which clear changes occur in the X-ray variability, X-ray spectral, or multi-wavelength properties.

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